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The Hidden Worlds of Quantum Mechanics

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Title: The Hidden Worlds of Quantum Mechanics


1
The Hidden Worlds of Quantum Mechanics
  • Craig Callender
  • Philosophy, UCSD
  • ccallender_at_ucsd.edu

2
Double Slit Experiment
3
(No Transcript)
4
What you would expect is
5
But what actually happens is
  • 1961, Jönsson, Zeitschrift für Physik 161 454
  • 1974, P. Merli, G. Missiroli and G. Pozzi in
    Bologna in 1974
  • Hitachi (A Tonomura et al). 1989 Demonstration of
    single-electron buildup of an interference
    pattern Am. J. Phys. 57

6
The Double Slit Experiment
7
Actual images
Bologna 1974
Hitachi 1989
8
(No Transcript)
9
Structure of Physical Theories
  • Stuff Newtonian corpuscles
  • State (xi, pi)
  • Dynamical law Hamiltons equations
  • Stuff ?
  • State wavefunction or vector ?gt
  • Dynamical law Schrodingers equation

10
Wave function (quantum state)
?(x)
x
11
?2(x) gives the probability of finding the
particle at position x
Most probable location of particle
?2(x)
x
12
where the observable is assumed to have a
discrete spectrum of eigenvalues, u are the
(normalized) eigenfunctions, and the coefficient
cn of the nth term gives the probability of the
nth eigenvalue via cn2.
13
Schrodinger evolution
Schrodinger evolution
?i(x)
?f(x)
  • Deterministic
  • Unitary
  • Linear

14
Three Ingredients for Trouble
  • Linear dynamical evolution
  • Eigenstate-eigenvalue rule
  • Determinate outcomes

15
Linearity
  • If the evolution takes Agt ?Bgt..
  • And takes Cgt ? Dgt
  • Then it takes the state
  • Agt Cgt ? Bgt Dgt

16
Eigenstate-eigenvalue link
  • A system in the quantum state ?gt has the value a
    for the observable  if and only if ?gt assigns
    the probability 1 to a and the probability 0 to
    all other possible values of Â.
  • Â ?gt a?gt

?(x)
x
17
Measurement
  • 1 readygtM?gtS ? upgtM?gtS
  • 2 readygtM?gtS ? downgtM?gtS
  • readygtM (a1?gtSa2?gtS)
  • a1readygtM?gtSa2readygtM?gtS
  • ? (a1upgtM?gtS a2downgtM?gtS)

18
Schrödingers cat
  • 1 cat readygtreadygtM?gtS ? cat deadgtupgtM?gtS
  • 2 cat readygtreadygtM?gtS ? cat
    alivegtdowngtM?gtS
  • cat readygtreadygtM (a1?gtS a2?gtS)
  • a1cat readygtreadygtM?gtS a2cat
    readygtreadygtM?gtS
  • ? (a1deadgtupgtM?gtS a2alivegtdowngtM?gtS

19
Measurement Problem
  • The quantum state is representationally complete,
    i.e., the eigenstate-eigenvalue link holds
  • The quantum state always evolves according to a
    linear laws of evolution, e.g., Schrodinger
    equation.
  • Measurements yield definite values
  • Contradiction!

20
Schrodinger evolution
?f(x)
?i(x)
Final state is a probability distribution but in
the real world something actually happens!
non-Schrodinger evolution miracle collapse
?i(x)
?f(x)
21
MP is Here to Stay
  • Quantum field theory employs superpositions among
    distinct macroscopic states
  • Theories on the horizon do too, e.g., superstring
    theory, loop theory, etc.
  • So MP has to be solved

22
The Standard Solution
  • Copenhagen (Bohr, Heisenberg, Dirac, von Neumann,
    )
  • Two types of evolution
  • Unmeasured evolution
  • Measurement evolution
  • Quantum philosophy of realism about
    macroscopic entities but anti-realism about
    microscopic ones

23
Unique?
  • Rosenfeld quantum theory eminently possess this
    character of uniqueness every feature of it has
    been forced upon us as the only way to avoid the
    ambiguities which would essentially affect any
    attempt at an analysis in classical terms of
    typical quantum phenomena

24
Criticism
  • It would seem that the theory is exclusively
    concerned about "results of measurement", and has
    nothing to say about anything else. What exactly
    qualifies some physical systems to play the role
    of "measurer"? Was the wavefunction of the world
    waiting to jump for thousands of millions of
    years until a single-celled living creature
    appeared? Or did it have to wait a little longer,
    for some better qualified system ... with a
    Ph.D.? If the theory is to apply to anything but
    highly idealized laboratory operations, are we
    not obliged to admit that more or less
    "measurement-like" processes are going on more or
    less all the time, more or less everywhere.

25
Solution Deny one of the premises
  1. The quantum state is representationally complete,
    i.e., the eigenstate-eigenvalue link holds
  2. The quantum state always evolves according to a
    linear laws of evolution, e.g., Schrodinger
    equation.
  3. Measurements yield definite values

26
Deny 1
  • Bohm-like hidden variable theories
  • De Broglie 1927
  • Bohm 1952
  • Bohm and Vigier
  • Nelsons stochastic mechanics
  • Bell 1987
  • Goldstein, Durr and Zanghi 1991

27
Deny 2
  • Physically-specifiable Collapse theories
  • Pearle 1989
  • Pearle and Squires 1994
  • Pearle 1996
  • Ghiradhi, Rimini and Weber 1986
  • Bell 1987
  • Penrose

28
Deny 3
  • Many-world type theories
  • Everett 1957
  • deWitt
  • Many minds
  • Barbour
  • Rovellis relational qm

29
Bohmian Mechanics
  • De Broglie 1927 David Bohm 1952
  • The de Broglie-Bohm idea seems so natural and
    simple, to resolve the wave-particle dilemma in
    such a clear and ordinary way, that it is a great
    mystery that it was so generally ignored. Bell,
    1987.

30
Bohmian Mechanics
  • Basic idea Suppose that there are some particles
    and that their velocities are determined by ?
    In other words, ? is not the whole story there
    are also particles.

31
Bohmian mechanics
Schrodinger equation
Velocity equation
at time t0
If
at time t
then
32
GRW
33
  • The world is described by two equations, the
    Schrodinger equation and the velocity equation.
    The latter is arguably the simplest first order
    equation for the positions of particles
    compatible with the Galilean and time reversal
    invariance of the former.
  • Given any probability distribution for the
    initial configuration, Bohmian mechanics defines
    a probability distribution for the full
    trajectory. Notice that the velocity equation is
    simply v J/p, where J is the quantum probability
    current and p is the quantum probability density.
    It follows from the quantum continuity equation
    that if the distribution of the configuration Q
    is given by psi at some time (say the initial
    time) this will be true at all times.
  • This deterministic theory of particles completely
    accounts for all the phenomena of nonrelativistic
    quantum mechanics, from interference effects to
    spectral lines. Thus Bohmian mechanics provides
    us with probabilities for complete
    configurational histories that are consistent
    with the quantum mechanical probabilities for
    configurations, including the positions of
    measuring devices.

34
Many Bohmian Theories
  • Deterministic alternatives to the velocity
    equation that are empirically adequate
  • Indeterministic versions of velocity equation
  • Spin as fundamental with position (Bohm, Schiller
    and Tiomno 1955, Dewdney 1992, Holland and Vigier
    1988, Bohm and Hiley 1993)
  • Bell-Bub-Vink dynamics discrete, indeterministic
  • Bub modal interpretation

35
Ghirardi, Rimini Weber 1986
  • Basic Idea The Schrodinger equation is not quite
    right. The wavefunction ?(r1,r2, ..., t) usually
    evolves according to the Schrodinger equation,
    but every now and then, at random, ? is
    multiplied (hit) by a gaussian function (and
    then normalized). How often the state is likely
    to be hit by a gaussian is proportional to how
    many particles there are in the system.
  • The effect of this multiplication is to collapse
    the state to a more localized one. Thus, systems
    with large N turn out to be overwhelmingly likely
    to collapse, and systems with small N turn out to
    be unlikely to collapse.

36
GRW
?(x)
x
Cat Alive
Cat Dead
1/?2(?C(r1,r2, ...rN...rM, t)??S(r1))
(?C(r1,r2, ...rN...rM, t)?? S(r1))
37
Then the Gaussian hits
?(x)
j(x) K exp (-x - ri2/2a2)
? j(x, ri)?(...,t)/ Ri(x).
x
Cat Alive
a10-5cm, jump time T1016s For N 1023,
collapse happens around 10-7s, compared to
observation time 10-2s
38
Many GRWs
  • Ghirardi emphasizes the importance of specifying
    what he calls the physical reality of what
    exists out there.''
  • Mass density interpretation for the simple GRW
    theory described here can be identified with the
    mass weighted sum, over all particles, of the
    one-particle densities arising from integrating
    over the coordinates of all but one of the
    particles.
  • Hit interpretation Bell p 205, that the
    space-time points (x,t) at which the hits are
    centered (which are determined by the wave
    function trajectory) should themselves serve as
    the local beables of the theory. These are the
    mathematical counterparts in the theory to real
    events at definite places and times in the real
    world (as distinct from the many purely
    mathematical constructions that occur in the
    working out of physical theories, as distinct
    from things which may be real but not localized,
    and as distinct from the observables' of other
    formulations of quantum mechanics, for which we
    have no use here.) A piece of matter then is a
    galaxy of such events.'
  • SL v CSL

39
Bohm GRW Everett
Deterministic? Yes No Yes
Time reversal invariant? Yes No Yes
Monistic? No Yes Yes
Particles? Yes No No
Is spin real? No Yes Yes
Preferred foliation? Yes Yes Maybe not
40
  • There is something wrong with all of these
    post-Copenhagen interpretationsthey dont offer
    new predictions
  • But
  • Why should when the theory is developed be
    important?
  • De Broglie 1927
  • GRW will differ from Copenhagen Bohm would if
    Copenhagen were clear plus, one never knows

41
Underdetermination of Theory by Evidence
THEORY1
THEORY2
Observable evidence
THEORY3
THEORY4
42
  • Duhem
  • Shall we ever dare to assert that no other
    hypothesis is imaginable? Light may be a swarm
    of projectiles, or it may be a vibratory motion
    whose waves are propagated in a medium is it
    forbidden to be anything else at all?
  • (1914)

43
Experimenta Crucis?
  • Bohm v Copenhagen
  • Times of arrival, etc.
  • Conroversial
  • Bohm v Everett
  • in principle underdetermination
  • Laudan and Leplin 1991
  • GRW v Bohm (or Copenhagen)
  • Localizations ? greater KE ? heating
  • Resistance of a superconductor different (Gallis
    Flemming Rae Rimini)
  • One mole of H one atom excited/sec
  • hope of reaching a crucial testextremely dim

44
Theoria crucis?
  • Solving the measurement problem seems to involve
    adding some new physics
  • The new physics may or may not be experimentally
    detectable in the future
  • But it might be crucial to new theories, e.g.,
    Bohmian quantum gravity, GRWs energy
    contribution, and so on.

45
Philosophers are any real theories
under-determined?
  • Our evidence is equally compatible with T (our
    best physical theory) and T (we and our
    apparently T-governed world is a computer
    simulation)
  • But T is just skepticism, not a real physical
    theory

46
Philosophers underdetermination too local to be
interesting?
The evidence equally supports T (newtonian
mechanics plus gravitational theory plus universe
is at rest in absolute space) and T (same, but
universe moving 5mph wrt absolute space)
5mph
47
How should we react in QM case?
48
Lesson of Quantum Mechanics Bad News
  • GRW, Bohm, Everett, etc. show that there is
    underdetermination by genuine scientific
    theories, contrary to what some philosophers
    suggest.
  • Furthermore, its hardly too local to care
    aboutit involves the central terms of our most
    fundamental theory
  • Real life is stranger than fiction or philosophy

49
Good news
  • Further testing may narrow down the available
    possibilities
  • Further theorizing may narrow down the
    possibilities
  • The UT doesnt seem to be of the kind that would
    challenge realist interpretations of most
    science.
  • First, one might appeal to non-observable facts,
    e.g., simplicity
  • Second, the underdetermination is not entirely
    general
  • Third, there are still levels that are not
    under-determined wrt the evidence, e.g., energy
    nuclear levels (Cordero 2002), scattering, etc.
  • Nevertheless, were stuck with a bewildering
    amount of underdetermination, like it or notso
    its best to learn to like it.
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